"The Contribution of Active Galactic Nuclei to the Diffuse Gamma Ray Background"

preprint1994arXivOpen access

Abstract

We consider the emission of high energy to very high energy γγ-rays in radio-quiet active galactic nuclei (AGN) or the central regions of radio-loud AGN. We use our results to estimate the γγ-ray flux from the central regions of nearby AGN, and then to calculate the contribution to the diffuse γγ-ray flux from unresolved AGN.

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